ChandraX-ray observations of the 3C 295 cluster core

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Chandra X - ray observations of the 3 C 295 cluster core

We examine the properties of the X-ray gas in the central regions of the distant (z = 0.46), X-ray luminous cluster of galaxies surrounding the powerful radio source 3C295, using observations made with the Chandra Observatory. Between radii of 50−500 kpc, the cluster gas is approximately isothermal with an emission-weighted temperature, kT ∼ 5 keV. Within the central 50 kpc radius this value dr...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 2001

ISSN: 0035-8711,1365-2966

DOI: 10.1046/j.1365-8711.2001.04315.x